Hostname: page-component-7479d7b7d-68ccn Total loading time: 0 Render date: 2024-07-10T04:31:01.441Z Has data issue: false hasContentIssue false
  • English
  • Français

Shaping bipolar and elliptical Planetary Nebulae: Rotation and magnetic field

Published online by Cambridge University Press:  25 May 2016

Guillermo García-Segura ,
Norbert Langer ,
Michał Różyczka ,
Mordechai-Mark Mac Low  and
José Franco
Guillermo García-Segura
Affiliation:
1Instituto de Astronomía-UNAM
Norbert Langer
Affiliation:
2Max-Planck-Institut für Astrophysik
Michał Różyczka
Affiliation:
3Warsaw University Observatory
Mordechai-Mark Mac Low
Affiliation:
4Max-Planck-Institut für Astronomie
José Franco
Affiliation:
1Instituto de Astronomía-UNAM

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present hydrodynamical and magnetohydronynamical simulations for the formation and evolution of bipolar and elliptical planetary nebulae with two interacting winds. The models are performed under the hypothesis of a single central source, i.e. binary systems are not considered and a single initial wind function is used in our calculations. We explore various relevant parameters, including the effects of stellar rotation, ionizing radiation field and stellar magnetic field, and a catalogue of resulting shapes is generated.

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 226
Copyright
Copyright © Kluwer 1997